Why do we need high-resolution observations of the Sun?

Details Why do we need high-resolution observations of the Sun? Why do we need high-resolution observations of the Sun?

Feb 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003spie.4853..453k&link_type=abstract

Innovative Telescopes and Instrumentation for Solar Astrophysics. Edited by Stephen L. Keil, Sergey V. Avakyan . Proceedings o

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

To make progress on major unsolved problems in solar physics (e.g., coronal heating, eruptive flare/CME initiation, solar wind initiation), we must observe on scales relevant to the underlying physical processes and their signatures. In this review I discuss the factors determining the structure of magnetic fields and plasmas in the Sun’s outer atmosphere, the key observable signatures of the relevant processes and properties, and the instrumental capabilities necessary to detect and measure these signatures. The primary emphasis is on state-of-the-art theoretical and numerical predictions, which often are the only means by which we can estimate the complex time-dependent evolution of the underlying physical mechanisms and their local and global effects on the corona.

Affiliated with

Also associated with

No associations

Rating

Why do we need high-resolution observations of the Sun? does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Why do we need high-resolution observations of the Sun?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Why do we need high-resolution observations of the Sun? will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-917121